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. 1999 Aug 3;96(16):9068–9073. doi: 10.1073/pnas.96.16.9068

Figure 2.

Figure 2

Stereo views of minimized average structures of high probability clusters at 300 K. (a) The most probable cluster (black) (10.7%) compared with the structure shown in Fig. 1 a (gray). (b–e) Clusters with overall rms deviations from the native structure of more than 3.0 Å.